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Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures
Zimovets, I. V.1; McLaughlin, J. A.2; Srivastava, A. K.3; Kolotkov, D. Y.4,5; Kuznetsov, A. A.6; Kupriyanova, E. G.7; Cho, I. -h.8; Inglis, A. R.9; Reale, F.10,11; Pascoe, D. J.12; Tian, H.13,14; Yuan, D.14,15; Li, D.16; Zhang, Q. M.16
2021-08-01
Source PublicationSPACE SCIENCE REVIEWS
ISSN0038-6308
Volume217Issue:5Pages:94
AbstractThe phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been known for over 50 years and significant progress has been made in this research area. It has become clear that QPPs are not rare-they are found in many flares and, therefore, robust flare models should reproduce their properties in a natural way. At least fifteen mechanisms/models have been developed to explain QPPs in solar flares, which mainly assume the presence of magnetohydrodynamic (MHD) oscillations in coronal structures (magnetic loops and current sheets) or quasi-periodic regimes of magnetic reconnection. We review the most important and interesting results on flare QPPs, with an emphasis on the results of recent years, and we present the predicted and prominent observational signatures of each of the fifteen mechanisms. However, it is not yet possible to draw an unambiguous conclusion as to the correct underlying QPP mechanism because of the qualitative, rather than quantitative, nature of most of the models and also due to insufficient observational information on the physical properties of the flare region, in particular the spatial structure of the QPP source. We also review QPPs in stellar flares, where progress is largely based on solar-stellar analogies, suggesting similarities in the physical processes in flare regions on the Sun and magnetoactive stars. The presence of QPPs with similar properties in solar and stellar flares is, in itself, a strong additional argument in favor of the likelihood of solar-stellar analogies. Hence, advancing our understanding of QPPs in solar flares provides an important additional channel of information about stellar flares. However, further work in both theory/simulations and in observations is needed.
KeywordSolar flares Stellar flares Quasi-periodic pulsations (QPPs) MHD oscillations MHD waves Magnetic reconnection
Funding OrganizationUK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA"
DOI10.1007/s11214-021-00840-9
WOS KeywordX-RAY PULSATIONS ; CORONAL LOOP OSCILLATIONS ; FREQUENCY OPTICAL OSCILLATIONS ; RECONNECTING CURRENT LAYER ; COHERENT RADIO-EMISSION ; CLASSICAL T TAURI ; DME FLARE ; PARTICLE-ACCELERATION ; MAGNETIC-FIELD ; WAVE-PROPAGATION
Language英语
Funding ProjectUK Science and Technology Facilities Council (STFC)[ST/T000384/1] ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant[ST/T000252/1] ; Russian Science Foundation[21-12-00195] ; National Natural Science Foundation of China (NSFC)[11825301] ; National Natural Science Foundation of China (NSFC)[11790304(11790300)] ; NSFC[11803005] ; NSFC[11911530690] ; Shenzhen Technology Project[JCYJ20180306172239618] ; National Research Foundation of Korea[NRF-2019R1C1C1006033] ; Korea Astronomy and Space Science Institute[2020-1-850-07] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme[724326] ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA"
Funding OrganizationUK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA" ; UK Science and Technology Facilities Council (STFC) ; UK Science and Technology Facilities Council (STFC) ; Ministry of Science and Higher Education of the Russian Federation ; Ministry of Science and Higher Education of the Russian Federation ; STFC consolidated grant ; STFC consolidated grant ; Russian Science Foundation ; Russian Science Foundation ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NSFC ; NSFC ; Shenzhen Technology Project ; Shenzhen Technology Project ; National Research Foundation of Korea ; National Research Foundation of Korea ; Korea Astronomy and Space Science Institute ; Korea Astronomy and Space Science Institute ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme ; C1 grant TRACEspace of Internal Funds KU Leuven ; C1 grant TRACEspace of Internal Funds KU Leuven ; Basic Research program "PLASMA" ; Basic Research program "PLASMA"
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000674632200001
PublisherSPRINGER
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/76629
Collection中国科学院国家天文台
Corresponding AuthorZimovets, I. V.
Affiliation1.Russian Acad Sci IKI, Space Res Inst, 84-32 Profsoyuznaya Str, Moscow 117997, Russia
2.Northumbria Univ, Newcastle Upon Tyne NE1 8ST, Tyne & Wear, England
3.Indian Inst Technol BHU, Dept Phys, Varanasi 221005, Uttar Pradesh, India
4.Univ Warwick, Phys Dept, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
5.RAS, Inst Solar Terr Phys SB, Irkutsk 664033, Russia
6.Inst Solar Terr Phys, Irkutsk 664033, Russia
7.RAS, Cent Astron Observ Pulkovo, Pulkovskoe Shosse 65, St Petersburg 196140, Russia
8.Kyung Hee Univ, 1732 Deogyeong Daero, Yongin 17104, Gyeonggi Do, South Korea
9.NASA, Solar Phys Lab, Heliophys Sci Div, Goddard Space Flight Ctr, Code 671, Greenbelt, MD 20771 USA
10.Univ Palermo, Dipartimento Fis & Chim, Piazza Parlamento 1, I-90134 Palermo, Italy
11.INAF, Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy
12.Katholieke Univ Leuven, Math Dept, Ctr Math Plasma Astrophys, Celestijnenlaan 200B Bus 2400, B-3001 Leuven, Belgium
13.Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
14.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China
15.Harbin Inst Technol, Inst Space Sci & Appl Technol, Shenzhen 518055, Guangdong, Peoples R China
16.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Sci, Nanjing 210034, Peoples R China
Recommended Citation
GB/T 7714
Zimovets, I. V.,McLaughlin, J. A.,Srivastava, A. K.,et al. Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures[J]. SPACE SCIENCE REVIEWS,2021,217(5):94.
APA Zimovets, I. V..,McLaughlin, J. A..,Srivastava, A. K..,Kolotkov, D. Y..,Kuznetsov, A. A..,...&Zhang, Q. M..(2021).Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures.SPACE SCIENCE REVIEWS,217(5),94.
MLA Zimovets, I. V.,et al."Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures".SPACE SCIENCE REVIEWS 217.5(2021):94.
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